| Start Date | Context | Status | Description |
|---|---|---|---|
| 2026-11-09 | hst_1372.pmap | latest | Delivering new ACS WFC bias, dark, CTE-dark, and sink pixel reference files for data taken from July 27th, 2026 through October 16, 2026. These files were regenerated with the updated reference file pipeline to correctly subtract the appropriate short dark from each anneal. The previously delivered files for the July 27, August 28, and September 22 anneals were produced before this correction, so the superdark and CTE-corrected superdark products did not reflect the proper short dark subtraction. They are being replaced so that the reference files for this period are consistent and built with the corrected processing. |
| 2026-11-02 | hst_1371.pmap | archived | Delivery of initializing rmap for the new STIS BLAZETAB reference file type. It applies only to the NUV and FUV-MAMA spectroscopic modes. Also delivering the first files of the new STIS BLAZETAB reference file type, which calculates the blaze function by observation date for a given Echelle mode. The modes affected will be NUV- and FUV-MAMA Echelle mode observations. Reprocessing would not need to occur until the HST pipeline build with the BLAZETAB code changes has been released. These files will also necessitate a restructuring of the STIS PHOTTAB reference files to be delivered after the next HST pipeline build installation, hstcal v3.3.0. |
| 2026-11-02 | hst_1369.pmap | archived | Delivery of new STIS CCD bias and dark reference files for CCD data taken between October 01 2026 through October 31 2026. The files were generated from data taken in the same time frame under STIS calibration programs 18158, and 18156. |
| 2026-10-29 | hst_1368.pmap | archived | The ACS WFC bias, dark, CTE dark, and sink files were generated following the ACS WFC anneal on October 19, 2026, and should be used to calibrate ACS WFC observations taken between September 22, 2026 and October 19, 2026. |